4.1.45. Warm: continuous photoionised absorption model¶
The warm model is a multi-component version of the xabs model. In
the warm model, we construct a model for a continuous distribution of
column density as a function of
. It is
in some sense comparable to the differential emission measure models
used to model the emission from multi-temperature gas. Here we have
absorption from multi-ionization gas. Depending upon the physics of the
source, this may be a better approximation than just the sum of a few
xabs components. A disadvantage of the model may be (but this also
depends upon the physics of the source), that all dynamical parameters
for each value of
are the same, like the outflow velocity
and turbulent broadening. If this appears to be the case in a given
source, one may of course avoid this problem by taking multiple,
non-overlapping warm components.
The model assumes a logarithmic grid of equidistant values of
, between a lower limit
and an upper limit
. For each of the grid points
, a value of
can be adjusted; here
is given as
evaluated at
, where the differential column density is assumed to be a
continuous function of
. At each intermediate point, the
value of
is then determined by doing cubic spline interpolation in the
–
space. In order not to consume too much
computer time, the step size for numerical integration
can be set. A typical, recommended value for this
(the default) is 0.2.
For more information on this model, the atomic data and parameters we refer to Different types of absorption models.
The parameters of the model are:
xil1
: xil2
: npol
: The number of grid points for the dxi
: step size for numerical integration f01...f19
: Values of
The following parameters are common to all our absorption models:
fcov
: The covering factor of the absorber. Default value: 1 (full
covering)v
: Root mean square velocity rms
: Rms velocity dv
: Velocity distance zv
: Average systematic velocity col
: File name for the photoionisation
balance parametersRecommended citation: Steenbrugge et al. (2005)